PDRs4All

Context . The infrared universe is dominated by emission from polycyclic aromatic hydrocarbons (PAHs) observed as aromatic infrared bands (AIBs). JWST has produced a rich trove of information on these PAH signatures. Aims . We aim to investigate the photochemical evolution of PAHs in photodissociation regions (PDRs), focusing on their molecular edge structures across key zones, including the H II region, the ionization front, the atomic PDR, the dissociation front, and the molecular PDR. Methods . We utilized JWST’s MIRI-MRS observations of the Orion Bar for the PDRs4All JWST Early Release Science program. We investigated the spectral and spatial characteristics of 10–15 µm AIBs. Results . The AIBs at 10.6, 10.8, 11.0, 11.2, 12.0, 12.7, 13.5, 14.0, and 14.2 µm share large-scale spatial morphologies, peaking in the atomic PDR and gradually declining with distance from the PDR surface. Correlations between the AIBs reveal that they are largely carried by PAHs. Profile variations and subcomponents of the 11.2 and 12.0 µm AIBs reveal a carrier that behaves independently of PAHs, which we attribute to very small grains (VSGs) and/or PAH clusters. We ascribe the 11.0 and 11.207 µm AIBs, part of the 12.0 µm AIB, and the 12.7, 13.5, and 14.2 µm AIBs to CH oop modes and discuss their hydrogen-adjacency assignments. We propose that the 10.6, 10.8, and 14.0 µm AIBs do not arise from CH oop modes. We derived the relative amounts of solo, duo, trio, and quartet CH groups to infer the molecular structures. These suggest that PAHs are dominated by solo and trio CH groups throughout the PDR. We attribute the decrease in duo and quartet CH groups relative to the solo CH groups toward the PDR surface to the effects of photolysis of the labile hydrogens. Conclusions . The 10–15 µm AIBs are powerful probes of the PAH molecular structures. This study showcases the spatial and spectral variability in CH oop features due to photochemical processing of PAHs, and the differentiated spectral characteristics of PAHs and VSGs, in a prototypical PDR.

Authors

Publication Details

Journal
Astronomy and Astrophysics
Published
2025-05-06
DOI
https://doi.org/10.1051/0004-6361/202554096
Citations
6
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
6.93

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

PDRs4All

Thomas S. -Y. Lai, E. Dartois, Takashi Onaka, Ryan Chown et al.
6 citations
Astronomy and Astrophysics
Astrophysics and Star Formation Studies
6.93
article

PDRs4All

Thomas S. -Y. Lai, E. Dartois, Takashi Onaka, Ryan Chown, Alyssa Sales, Ilane Schroetter, Alvaro Labiano, Bethany Schefter, Alessandra Ricca, Felipe Alarcón, Olivier Berné, E. Peeters, Boris Trahin, Mridusmita Buragohain, Amélie Canin, Yong Zhang, E. Habart, Alessandra Candian, Alexandros Maragkoudakis, Dries Van De Putte, Ameek Sidhu, Olga Kannavou, Christiaan Boersma, B. P. Abbott, J. Cami, Baria Khan, R. Javier Goicoechea, G.M. Alexander Tielens
article en
6 citations

Abstract

Context . The infrared universe is dominated by emission from polycyclic aromatic hydrocarbons (PAHs) observed as aromatic infrared bands (AIBs). JWST has produced a rich trove of information on these PAH signatures. Aims . We aim to investigate the photochemical evolution of PAHs in photodissociation regions (PDRs), focusing on their molecular edge structures across key zones, including the H II region, the ionization front, the atomic PDR, the dissociation front, and the molecular PDR. Methods . We utilized JWST’s MIRI-MRS observations of the Orion Bar for the PDRs4All JWST Early Release Science program. We investigated the spectral and spatial characteristics of 10–15 µm AIBs. Results . The AIBs at 10.6, 10.8, 11.0, 11.2, 12.0, 12.7, 13.5, 14.0, and 14.2 µm share large-scale spatial morphologies, peaking in the atomic PDR and gradually declining with distance from the PDR surface. Correlations between the AIBs reveal that they are largely carried by PAHs. Profile variations and subcomponents of the 11.2 and 12.0 µm AIBs reveal a carrier that behaves independently of PAHs, which we attribute to very small grains (VSGs) and/or PAH clusters. We ascribe the 11.0 and 11.207 µm AIBs, part of the 12.0 µm AIB, and the 12.7, 13.5, and 14.2 µm AIBs to CH oop modes and discuss their hydrogen-adjacency assignments. We propose that the 10.6, 10.8, and 14.0 µm AIBs do not arise from CH oop modes. We derived the relative amounts of solo, duo, trio, and quartet CH groups to infer the molecular structures. These suggest that PAHs are dominated by solo and trio CH groups throughout the PDR. We attribute the decrease in duo and quartet CH groups relative to the solo CH groups toward the PDR surface to the effects of photolysis of the labile hydrogens. Conclusions . The 10–15 µm AIBs are powerful probes of the PAH molecular structures. This study showcases the spatial and spectral variability in CH oop features due to photochemical processing of PAHs, and the differentiated spectral characteristics of PAHs and VSGs, in a prototypical PDR.

Astronomy and AstrophysicsVol. 699
National Aeronautics and Space Administration, Canadian Space Agency, Japan Society for the Promotion of Science
Openalex Percentile: Top 3%
Astrophysics and Star Formation Studies
6.93
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.